We present a model to explain the decrease in the amplitude of the pul
se profile with increasing energy observed in Geminga's soft X-ray sur
face thermal emission. We assume the presence of plates surrounded by
a surface with very distinct physical properties: these two regions em
it spectra of very distinct shapes which present a crossover, the warm
plates emitting a softer spectrum than the colder surrounding surface
. The strongly pulsed emission from the plates dominates at low energy
while the surrounding's emission dominates at high energy, producing
naturally a strong decrease in the pulsed fraction. In our illustrativ
e example, the plates are assumed to be magnetized, while the rest of
the surface is field free. This plate structure may be seen as a schem
atic representation of a continuous but very nonuniform distribution o
f the surface magnetic field or as a quasi-realistic structure induced
by past tectonic activity on Geminga.